Technique

Halo Effect and Bloom in Night Vision: Explained Simply

August 20263 min read

Halo Effect and Bloom in Night Vision: Explained Simply

You're out in the field, tube powered on, when a vehicle's headlights sweep across your field of view in the distance. A moment later, part of the image disappears under a milky glare. This isn't a manufacturing flaw or a malfunction — it's your tube encountering two well-known phenomena among night vision users: halo and bloom. Two terms that are often mixed up, even though they describe two distinct mechanisms inside the image intensifier tube.

What happens inside a tube

To understand halo and bloom, we need to go back to the basic principle of light intensification. The photocathode converts incoming photons into electrons. These electrons are then multiplied by the Microchannel Plate (MCP) before striking a phosphor screen, which renders the image you see through the eyepiece — typically in green (P43) or white (P45).

This process works remarkably well under low ambient light: starlight, moonlight, reflections off vegetation. The problem arises when a bright, point-source light — headlights, a flashlight, a lit window — strikes a very localized area of the photocathode.

Halo: a localized optical artifact

Halo is the bright, often tinted ring that surrounds an intense light source in the image. It comes from light scattering inside the tube itself: some of the electrons generated at the point where the bright light hits the photocathode spread laterally before reaching the phosphor screen, creating a blurred circle around the point source.

This effect is purely optical and localized — it only affects the immediate area around the bright source. The rest of the image stays readable. It's an artifact that every microchannel-plate tube deals with, including the high-end NNVT tubes we distribute.

Bloom: a global, temporary saturation

Bloom is a different phenomenon, and often more disruptive in the field. When the amount of light hitting the tube far exceeds its processing capacity, the entire image — not just the area around the source — saturates in brightness. The whole frame whites out, surrounding detail disappears, and a temporary blinding effect sets in until the tube regains its balance.

Bloom is therefore a global, time-based effect, while halo is a local and largely persistent one for as long as the light source stays within the field of view.

Autogating: the technical answer to bloom

Autogating technology was developed specifically to limit bloom. An autogated tube pulses the power supplied to the microchannel plate at extremely high frequency, based on detected ambient brightness. When a sudden bright source appears, the voltage is cut or reduced thousands of times per second, which significantly limits overall image saturation and speeds up the return to a usable image.

The NNVT tubes we integrate into our LNVM and LAB-NVS housings benefit from this technology — something we cover in more depth in our article on FOM, SNR, and Autogating.

Can halo and bloom be eliminated entirely?

No — and that's worth knowing before you buy. No light-intensification tube, regardless of price or generation, is fully immune to either phenomenon. These are physical limitations inherent to analog photomultiplication technology. What separates a good tube from a mediocre one is the intensity of the effect and the speed of recovery, not its outright disappearance.

A few habits can limit their impact in the field:

  • Avoid looking directly at an intense light source whenever possible
  • Choose an autogated tube for use in semi-urban or roadside environments
  • Anticipate known light sources (headlights, street lighting) rather than being caught off guard by them in your field of view

The takeaway

Halo is the ring around a bright light. Bloom is the glare that overtakes the whole image. Two different consequences of the same underlying challenge: combining extreme sensitivity to low light with the occasional presence of far brighter sources. Understanding this distinction helps you choose a better tube — and read what you're seeing through the eyepiece as physics, not as a flaw.